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Fig. A.1.

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Evolution of the metallicity profile with mass coordinate. The solid blue and dashed gray lines show the K2-MZvar-A2-12 and K2-A2-12 models, respectively, at 10 Myr (end of the accretion phase; panel a), 100 Myr (b), 1 Gyr (c), and 4.567 Gyr (solar age; d). Animations showing the metallicity profile in the solar interior of these models are available online and at Zenodo.

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